Planet Kepler-62 b
| Name | Kepler-62 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2013 | ||
| Mass | 0.028 ( -0.028 +0.0 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0553 (± 0.0005) AU | |
|
| Orbital Period | 5.714932 (± 9e-06) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.117 ( -0.0036 +0.0036 ) RJ | |
|
| Inclination | 89.2 (± 0.4) deg | |
|
| Update | 2014-05-22 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | 2455003.9189 (± 0.0009) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
Kepler-62| Name | Kepler-62 | ||
| Distance | — | ||
| Spectral type | K2V | ||
| Apparent magnitude V | 14.0 | ||
| Mass | 0.69 (± 0.02) MSun | ||
| Age | — | ||
| Effective temperature | 4869.0 K | ||
| Radius | 0.63 (± 0.02) RSun | ||
| Metallicity [Fe/H] | -0.21 | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 18:52:51.0 | ||
| Dec2000 | +45:20:60 | ||
| Alternate Names | |||
| Planetary system | 5 planets |
Observability Predictor 
Remarks
The planet mass upper limit is not inferred from RV measurements but from the planet radius and a planet model (Borucki et al. 2013).Related publications
Exo-Milankovitch Cycles I: Orbits and Rotation States
2018
DEITRICK R., BARNES R., QUINN Th., ARMSTRONG J., CHARNEY B. & WILHELM C.
Astron. J., 155, 60
paper arxiv
How alien can alien worlds be?
2017
ADIBEKYAN F., FIGUEIRA P. & SANTOS N.
in EWASS Special Session 4 (2017): Star-planet interactions
arxiv
Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11
2016
MIA R. & KUSHVAH B.
MNRAS, 457, 1089
paper arxiv
Gravitational quantization of exoplanet orbits in HD 40307, $μ$ Ara, Kepler-26, Kepler-62, and Kepler-275: Comparing predicted orbits
2015
GEROYANNIS V.
arxiv
Mercury-T: A new code to study tidally evolving multi-planet systems. Applications to Kepler-62
2015
BOLMONT E., RAYMOND S., LECONTE J., HERSANT F. & CORREIA A.
Astron. & Astrophys., accepted
arxiv
Habitable Zone Dependence on Stellar Parameter Uncertainties
2014
KANE S.
ApJ, 782, 111
paper arxiv
Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186
2014
BOLMONT E., RAYMOND S., LECONTE J., CORREIA A. & QUINTANA E.
in IAU Symposium No. 310
arxiv
Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone
2013
BORUCKI W., AGOL E., FRESSIN F., KALTENEGGER L., ROWE J. & 59 additional authors
Science, 340, 587
paper arxiv
